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Physical parameterization of Strombolian eruptions via experimentally-validated modeling of high-speed observations

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Physical parameterization of Strombolian eruptions via experimentally-validated modeling of high-speed observations. / Taddeucci, Jacopo; Alatorre-Ibarguengoitia, Miguel; Moroni, Monica et al.
In: Geophysical Research Letters, Vol. 39, No. 16, L16306, 23.08.2012.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Taddeucci, J, Alatorre-Ibarguengoitia, M, Moroni, M, Tornetta, L, Capponi, A, Scarlato, P, Dingwell, D & De Rita, D 2012, 'Physical parameterization of Strombolian eruptions via experimentally-validated modeling of high-speed observations', Geophysical Research Letters, vol. 39, no. 16, L16306. https://doi.org/10.1029/2012GL052772

APA

Taddeucci, J., Alatorre-Ibarguengoitia, M., Moroni, M., Tornetta, L., Capponi, A., Scarlato, P., Dingwell, D., & De Rita, D. (2012). Physical parameterization of Strombolian eruptions via experimentally-validated modeling of high-speed observations. Geophysical Research Letters, 39(16), Article L16306. https://doi.org/10.1029/2012GL052772

Vancouver

Taddeucci J, Alatorre-Ibarguengoitia M, Moroni M, Tornetta L, Capponi A, Scarlato P et al. Physical parameterization of Strombolian eruptions via experimentally-validated modeling of high-speed observations. Geophysical Research Letters. 2012 Aug 23;39(16):L16306. doi: 10.1029/2012GL052772

Author

Taddeucci, Jacopo ; Alatorre-Ibarguengoitia, Miguel ; Moroni, Monica et al. / Physical parameterization of Strombolian eruptions via experimentally-validated modeling of high-speed observations. In: Geophysical Research Letters. 2012 ; Vol. 39, No. 16.

Bibtex

@article{54a773a38dad47fa8eddbf21bc31b22f,
title = "Physical parameterization of Strombolian eruptions via experimentally-validated modeling of high-speed observations",
abstract = "Pressurized gas drives explosive volcanic eruptions.Existing models can predict the amount and pressure of gas in erupting magma, but application and testing of such models is currently limited by the accuracy of input parameters from natural systems. Here, we present a new methodology,based on a novel integration of 1) high-speed imaging and 2) shock-tube modeling of volcanic activity in order to derive estimates of sub-second variations in the pressure, mass, and volume of gas that drive the dynamics of unsteadyeruptions. First, we validate the method against laboratoryscale shock-tube experiments. Having validated the method we then apply it to observations of eruptions at Stromboli volcano (Italy). Finally, we use those results for a parametric study of the weight of input parameters on final outputs. Weconclude that Strombolian explosions, with durations of seconds, result from discrete releases of gas with mass and pressure in the 4–714 kg and 0.10–0.56 MPa range, respectively, and which occupy the volcano conduit to a depth of4–190 m. These variations are present both among and within individual explosions",
author = "Jacopo Taddeucci and Miguel Alatorre-Ibarguengoitia and Monica Moroni and Lauretta Tornetta and Antonio Capponi and Piergiorgio Scarlato and Donald Dingwell and {De Rita}, Donatella",
year = "2012",
month = aug,
day = "23",
doi = "10.1029/2012GL052772",
language = "English",
volume = "39",
journal = "Geophysical Research Letters",
issn = "0094-8276",
publisher = "John Wiley & Sons, Ltd",
number = "16",

}

RIS

TY - JOUR

T1 - Physical parameterization of Strombolian eruptions via experimentally-validated modeling of high-speed observations

AU - Taddeucci, Jacopo

AU - Alatorre-Ibarguengoitia, Miguel

AU - Moroni, Monica

AU - Tornetta, Lauretta

AU - Capponi, Antonio

AU - Scarlato, Piergiorgio

AU - Dingwell, Donald

AU - De Rita, Donatella

PY - 2012/8/23

Y1 - 2012/8/23

N2 - Pressurized gas drives explosive volcanic eruptions.Existing models can predict the amount and pressure of gas in erupting magma, but application and testing of such models is currently limited by the accuracy of input parameters from natural systems. Here, we present a new methodology,based on a novel integration of 1) high-speed imaging and 2) shock-tube modeling of volcanic activity in order to derive estimates of sub-second variations in the pressure, mass, and volume of gas that drive the dynamics of unsteadyeruptions. First, we validate the method against laboratoryscale shock-tube experiments. Having validated the method we then apply it to observations of eruptions at Stromboli volcano (Italy). Finally, we use those results for a parametric study of the weight of input parameters on final outputs. Weconclude that Strombolian explosions, with durations of seconds, result from discrete releases of gas with mass and pressure in the 4–714 kg and 0.10–0.56 MPa range, respectively, and which occupy the volcano conduit to a depth of4–190 m. These variations are present both among and within individual explosions

AB - Pressurized gas drives explosive volcanic eruptions.Existing models can predict the amount and pressure of gas in erupting magma, but application and testing of such models is currently limited by the accuracy of input parameters from natural systems. Here, we present a new methodology,based on a novel integration of 1) high-speed imaging and 2) shock-tube modeling of volcanic activity in order to derive estimates of sub-second variations in the pressure, mass, and volume of gas that drive the dynamics of unsteadyeruptions. First, we validate the method against laboratoryscale shock-tube experiments. Having validated the method we then apply it to observations of eruptions at Stromboli volcano (Italy). Finally, we use those results for a parametric study of the weight of input parameters on final outputs. Weconclude that Strombolian explosions, with durations of seconds, result from discrete releases of gas with mass and pressure in the 4–714 kg and 0.10–0.56 MPa range, respectively, and which occupy the volcano conduit to a depth of4–190 m. These variations are present both among and within individual explosions

U2 - 10.1029/2012GL052772

DO - 10.1029/2012GL052772

M3 - Journal article

VL - 39

JO - Geophysical Research Letters

JF - Geophysical Research Letters

SN - 0094-8276

IS - 16

M1 - L16306

ER -